Radar data obtained from Arecibo and Goldstone along with photometry obtained from the Panchromatic Robotic Monitoring and Polarimetry telescopes (PROMPT) in Chile in June 2009 are used to construct a three-dimensional shape model of near-Earth asteroid (136617) 1994 CC as reported by Brozovic et al. (2011).  The radar data reveal (136617) 1994 CC is a triple system, but only the primary body has a 3-D shape model due to the lack of resolution and rotational coverage of the satellites.  The model provides a good match to the image resolution of 19 m, an effective diameter of 0.62 +/- 0.06 km, and a sidereal rotation period of 2.3886 +/- 0.0001 h.



REFERENCES 
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Brozovic, M., L.A.M. Benner, P.A. Taylor, M.C. Nolan, E.S. Howell, C. Magri, D.J. Scheeres, J.D. Giorgini, J.T. Pollock, P. Pravec, A. Galad, J. Fang, J.L. Margot, M.W. Busch, M.K. Shepard, D.E. Reichart, K.M. Ivarsen, J.B. Haislip, A.P. LaCluyze, J. Jao, M.A. Slade, K.J. Lawrence, M.D. Hicks, Radar and optical observations and physical modeling of triple near-Earth asteroid (136617) 1994 CC, Icarus, 216, 241-256, 2011, doi:10.1016/j.icarus.2011.09.002.